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Browsing by Author "Chapman, S. C."
Now showing items 1-20 of 37
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Hezaveh, Y. D.; Marrone, D. P.; Fassnacht, C. D.; Spilker, J. S.; Vieira, J. D.; Aguirre, J. E.; Aird, K. A.; Aravena, M.; Ashby, Matthew L. N.; Bayliss, M.; Benson, B. A.; Bleem, L. E.; Bothwell, M.; Brodwin, M.; Carlstrom, J. E.; Chang, C. L.; Chapman, S. C.; Crawford, T. M.; Crites, A. T.; De Breuck, C.; de Haan, T.; Dobbs, M. A.; Fomalont, E. B.; George, E. M.; Gladders, M. D.; Gonzalez, A. H.; Greve, T. R.; Halverson, N. W.; High, F. W.; Holder, G. P.; Holzapfel, W. L.; Hoover, S.; Hrubes, J. D.; Husband, K.; Hunter, T. R.; Keisler, R.; Lee, A. T.; Leitch, E. M.; Lueker, M.; Luong-Van, D.; Malkan, M.; McIntyre, V.; McMahon, J. J.; Mehl, J.; Menten, K. M.; Meyer, S. S.; Mocanu, L. M.; Murphy, E. J.; Natoli, T.; Padin, S.; Plagge, T.; Reichardt, C. L.; Rest, A.; Ruel, J.; Ruhl, J. E.; Sharon, K.; Schaffer, K. K.; Shaw, L.; Shirokoff, E.; Stalder, B.; Staniszewski, Z.; Stark, Antony A.; Story, K.; Vanderlinde, K.; Weiß, A.; Welikala, N.; Williamson, R. (2013)We present Atacama Large Millimeter/submillimeter Array (ALMA) 860 µm imaging of four high-redshift (z = 2.8-5.7) dusty sources that were detected using the South Pole Telescope (SPT) at 1.4 mm and are not seen in existing ...
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Weiß, A.; De Breuck, C.; Marrone, D. P.; Vieira, J. D.; Aguirre, J. E.; Aird, K. A.; Aravena, M.; Ashby, Matthew L. N.; Bayliss, M.; Benson, B. A.; Béthermin, M.; Biggs, A. D.; Bleem, L. E.; Bock, J. J.; Bothwell, M.; Bradford, C. M.; Brodwin, M.; Carlstrom, J. E.; Chang, C. L.; Chapman, S. C.; Crawford, T. M.; Crites, A. T.; de Haan, T.; Dobbs, M. A.; Downes, T. P.; Fassnacht, C. D.; George, E. M.; Gladders, M. D.; Gonzalez, A. H.; Greve, T. R.; Halverson, N. W.; Hezaveh, Y. D.; High, F. W.; Holder, G. P.; Holzapfel, W. L.; Hoover, S.; Hrubes, J. D.; Husband, K.; Keisler, R.; Lee, A. T.; Leitch, E. M.; Lueker, M.; Luong-Van, D.; Malkan, M.; McIntyre, V.; McMahon, J. J.; Mehl, J.; Menten, K. M.; Meyer, S. S.; Murphy, E. J.; Padin, S.; Plagge, T.; Reichardt, C. L.; Rest, A.; Rosenman, M.; Ruel, J.; Ruhl, J. E.; Schaffer, K. K.; Shirokoff, E.; Spilker, J. S.; Stalder, B.; Staniszewski, Z.; Stark, Antony A.; Story, K.; Vanderlinde, K.; Welikala, N.; Williamson, R. (2013)Using the Atacama Large Millimeter/submillimeter Array, we have conducted a blind redshift survey in the 3 mm atmospheric transmission window for 26 strongly lensed dusty star-forming galaxies (DSFGs) selected with the ...
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Béthermin, M.; De Breuck, C.; Gullberg, B.; Aravena, M.; Bothwell, M. S.; Chapman, S. C.; Gonzalez, A. H.; Greve, T. R.; Litke, K.; Ma, J.; Malkan, M.; Marrone, D. P.; Murphy, E. J.; Spilker, J. S.; Stark, Antony A.; Strandet, M.; Vieira, J. D.; Weiß, A.; Welikala, N. (2016)We present ALMA detections of the [NII] 205 µm and CO(12-11) emission lines, and the tentative detection of [CI] - for the strongly lensed (µ = 5.7 ± 0.5) dusty, star-forming galaxy SPT-S J213242-5802.9 (hereafter SPT2132-58) ...
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Cunningham, D. J. M.; Chapman, S. C.; Aravena, M.; De Breuck, C.; Béthermin, M.; Chen, Chian-Chou; Dong, Chenxing; Gonzalez, A. H.; Greve, T. R.; Litke, K. C.; Ma, J.; Malkan, M.; Marrone, D. P.; Miller, T.; Phadke, K. A.; Reuter, C.; Rotermund, K.; Spilker, J. S.; Stark, Anthony A.; Strandet, M.; Vieira, J. D.; Weiß, A. (2020)We present Atacama Compact Array and Atacama Pathfinder Experiment observations of the [N II] 205 µm fine-structure line in 40 sub- millimetre galaxies lying at redshifts z = 3-6, drawn from the 2500 deg<SUP>2</SUP> South ...
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Reuter, C.; Vieira, J. D.; Spilker, J. S.; Weiss, A.; Aravena, M.; Archipley, M.; Béthermin, M.; Chapman, S. C.; De Breuck, C.; Dong, C.; Everett, W. B.; Fu, J.; Greve, T. R.; Hayward, C. C.; Hill, R.; Hezaveh, Y.; Jarugula, S.; Litke, K.; Malkan, M.; Marrone, D. P.; Narayanan, D.; Phadke, K. A.; Stark, Antony A.; Strandet, M. L. (2020)The South Pole Telescope (SPT) has systematically identified 81 high-redshift, strongly gravitationally lensed, dusty star-forming galaxies (DSFGs) in a 2500 square degree cosmological millimeter-wave survey. We present ...
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Riseley, C. J.; Scaife, A. M. M.; Hales, C. A.; Harrison, I.; Birkinshaw, M.; Battye, R. A.; Beswick, R. J.; Brown, M. L.; Casey, C. M.; Chapman, S. C.; Demetroullas, C.; Hung, C. -L; Jackson, N. J.; Muxlow, T.; Watson, B. (2016)We present the results of 325 MHz Giant Metrewave Radio Telescope observations of a supercluster field, known to contain five Abell clusters at redshift z 0.2. We achieve a nominal sensitivity of 34 µJy beam<SUP>-1</SUP> ...
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Béthermin, M.; Greve, T. R.; De Breuck, C.; Vieira, J. D.; Aravena, M.; Chapman, S. C.; Chen, Chian-Chou; Dong, C.; Hayward, C. C.; Hezaveh, Y.; Marrone, D. P.; Narayanan, D.; Phadke, K. A.; Reuter, C. A.; Spilker, J. S.; Stark, Antony A.; Strandet, M. L.; Weiß, A. (2018)The origin of the high star formation rates (SFR) observed in high-redshift dusty star-forming galaxies is still unknown. Large fractions of dense molecular gas might provide part of the explanation, but there are few ...
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Riechers, Dominik A.; Bradford, C. M.; Clements, D. L.; Dowell, C. D.; Pérez-Fournon, I.; Ivison, R. J.; Bridge, C.; Conley, A.; Fu, Hai; Vieira, J. D.; Wardlow, J.; Calanog, J.; Cooray, A.; Hurley, P.; Neri, R.; Kamenetzky, J.; Aguirre, J. E.; Altieri, B.; Arumugam, V.; Benford, D. J.; Béthermin, M.; Bock, J.; Burgarella, D.; Cabrera-Lavers, A.; Chapman, S. C.; Cox, P.; Dunlop, J. S.; Earle, L.; Farrah, D.; Ferrero, P.; Franceschini, A.; Gavazzi, R.; Glenn, J.; Solares, E. A. Gonzalez; Gurwell, M. A.; Halpern, M.; Hatziminaoglou, E.; Hyde, A.; Ibar, E.; Kovács, A.; Krips, M.; Lupu, R. E.; Maloney, P. R.; Martinez-Navajas, P.; Matsuhara, H.; Murphy, E. J.; Naylor, B. J.; Nguyen, H. T.; Oliver, S. J.; Omont, A.; Page, M. J.; Petitpas, Glen R.; Rangwala, N.; Roseboom, I. G.; Scott, D.; Smith, A. J.; Staguhn, J. G.; Streblyanska, A.; Thomson, A. P.; Valtchanov, I.; Viero, M.; Wang, L.; Zemcov, M.; Zmuidzinas, J. (2013)Massive present-day early-type (elliptical and lenticular) galaxies probably gained the bulk of their stellar mass and heavy elements through intense, dust-enshrouded starbursts--that is, increased rates of star formation--in ...
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Vieira, J. D.; Marrone, D. P.; Chapman, S. C.; De Breuck, C.; Hezaveh, Y. D.; Weiß, A.; Aguirre, J. E.; Aird, K. A.; Aravena, M.; Ashby, Matthew L. N.; Bayliss, M.; Benson, B. A.; Biggs, A. D.; Bleem, L. E.; Bock, J. J.; Bothwell, M.; Bradford, C. M.; Brodwin, M.; Carlstrom, J. E.; Chang, C. L.; Crawford, T. M.; Crites, A. T.; de Haan, T.; Dobbs, M. A.; Fomalont, E. B.; Fassnacht, C. D.; George, E. M.; Gladders, M. D.; Gonzalez, A. H.; Greve, T. R.; Gullberg, B.; Halverson, N. W.; High, F. W.; Holder, G. P.; Holzapfel, W. L.; Hoover, S.; Hrubes, J. D.; Hunter, T. R.; Keisler, R.; Lee, A. T.; Leitch, E. M.; Lueker, M.; Luong-van, D.; Malkan, M.; McIntyre, V.; McMahon, J. J.; Mehl, J.; Menten, K. M.; Meyer, S. S.; Mocanu, L. M.; Murphy, E. J.; Natoli, T.; Padin, S.; Plagge, T.; Reichardt, C. L.; Rest, A.; Ruel, J.; Ruhl, J. E.; Sharon, K.; Schaffer, K. K.; Shaw, L.; Shirokoff, E.; Spilker, J. S.; Stalder, B.; Staniszewski, Z.; Stark, Antony A.; Story, K.; Vanderlinde, K.; Welikala, N.; Williamson, R. (2013)In the past decade, our understanding of galaxy evolution has been revolutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant in the early Universe than at present. It has, ...
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Riechers, Dominik A.; Cooray, A.; Omont, A.; Neri, R.; Harris, A. I.; Baker, A. J.; Cox, P.; Frayer, D. T.; Carpenter, J. M.; Auld, R.; Aussel, H.; Beelen, A.; Blundell, R.; Bock, J.; Brisbin, D.; Burgarella, D.; Chanial, P.; Chapman, S. C.; Clements, D. L.; Conley, A.; Dowell, C. D.; Eales, S.; Farrah, D.; Franceschini, A.; Gavazzi, R.; Glenn, J.; Griffin, M.; Gurwell, M.; Ivison, R. J.; Kim, S.; Krips, M.; Mortier, A. M. J.; Oliver, S. J.; Page, M. J.; Papageorgiou, A.; Pearson, C. P.; Pérez-Fournon, I.; Pohlen, M.; Rawlings, J. I.; Raymond, G.; Rodighiero, G.; Roseboom, I. G.; Rowan-Robinson, M.; Scott, K. S.; Seymour, N.; Smith, A. J.; Symeonidis, M.; Tugwell, K. E.; Vaccari, M.; Vieira, J. D.; Vigroux, L.; Wang, L.; Wardlow, J.; Wright, G. (2011)We report the detection of CO(J = 5 ? 4), CO(J = 3 ? 2), and CO(J = 1 ? 0) emission in the strongly lensed, Herschel/SPIRE-selected submillimeter galaxy (SMG) HERMES J105751.1+573027 at z = 2.9574 ± 0.0001, using the Plateau ...
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Zavala, J. A.; Yun, M. S.; Aretxaga, I.; Hughes, D. H.; Wilson, G. W.; Geach, J. E.; Egami, E.; Gurwell, M. A.; Wilner, D. J.; Smail, Ian; Blain, A. W.; Chapman, S. C.; Coppin, K. E. K.; Dessauges-Zavadsky, M.; Edge, A. C.; Montaña, A.; Nakajima, K.; Rawle, T. D.; Sánchez-Argüelles, D.; Swinbank, A. M.; Webb, T. M. A.; Zeballos, M. (2015)We present Early Science observations with the Large Millimeter Telescope, AzTEC 1.1 mm continuum images and wide bandwidth spectra (73-111 GHz) acquired with the Redshift Search Receiver, towards four bright lensed ...
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Bussmann, R. S.; Riechers, D.; Fialkov, A.; Scudder, J.; Hayward, C. C.; Cowley, W. I.; Bock, J.; Calanog, J.; Chapman, S. C.; Cooray, A.; De Bernardis, F.; Farrah, D.; Fu, Hai; Gavazzi, R.; Hopwood, R.; Ivison, R. J.; Jarvis, M.; Lacey, C.; Loeb, A.; Oliver, S. J.; Pérez-Fournon, I.; Rigopoulou, D.; Roseboom, I. G.; Scott, Douglas; Smith, A. J.; Vieira, J. D.; Wang, L.; Wardlow, J. (2015)Not Available Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
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Spilker, J. S.; Aravena, M.; Béthermin, M.; Chapman, S. C.; Chen, C. -C; Cunningham, D. J. M.; De Breuck, C.; Dong, C.; Gonzalez, A. H.; Hayward, C. C.; Hezaveh, Y. D.; Litke, K. C.; Ma, J.; Malkan, M.; Marrone, D. P.; Miller, T. B.; Morningstar, W. R.; Narayanan, D.; Phadke, K. A.; Sreevani, J.; Stark, Antony A.; Vieira, J. D.; Weiß, A. (2018)Galaxies grow inefficiently, with only a small percentage of the available gas converted into stars each free-fall time. Feedback processes, such as outflowing winds driven by radiation pressure, supernovae, or supermassive ...
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Willner, Steven P.; Ashby, Matthew L. N.; Barmby, P.; Chapman, S. C.; Coil, A. L.; Cooper, M. C.; Huang, J. -S; Ivison, R.; Koo, D. C. (2012)Infrared 3.6-8 ?m images of the Extended Groth Strip yield plausible counterpart identifications for all but one of 510 radio sources in the AEGIS20 S(1.4 GHz) > 50 ?Jy sample. This is the first such deep sample that ...
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Marrone, D. P.; Spilker, J. S.; Hayward, C. C.; Vieira, J. D.; Aravena, M.; Ashby, M. L. N.; Bayliss, M. B.; Béthermin, M.; Brodwin, M.; Bothwell, M. S.; Carlstrom, J. E.; Chapman, S. C.; Chen, Chian-Chou; Crawford, T. M.; Cunningham, D. J. M.; De Breuck, C.; Fassnacht, C. D.; Gonzalez, A. H.; Greve, T. R.; Hezaveh, Y. D.; Lacaille, K.; Litke, K. C.; Lower, S.; Ma, J.; Malkan, M.; Miller, T. B.; Morningstar, W. R.; Murphy, E. J.; Narayanan, D.; Phadke, K. A.; Rotermund, K. M.; Sreevani, J.; Stalder, B.; Stark, Antony A.; Strandet, M. L.; Tang, M.; Weiß, A. (2018)According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in regions corresponding to the largest fluctuations ...
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Boselli, A.; Boissier, S.; Heinis, S.; Cortese, L.; Ilbert, O.; Hughes, T.; Cucciati, O.; Davies, J.; Ferrarese, L.; Giovanelli, R.; Haynes, M. P.; Baes, M.; Balkowski, C.; Brosch, N.; Chapman, S. C.; Charmandaris, Vassilis; Clemens, M. S.; Dariush, A.; de Looze, I.; di Serego Alighieri, S.; Duc, P. A.; Durrell, P. R.; Emsellem, E.; Erben, T.; Fritz, J.; Garcia-Appadoo, D. A.; Gavazzi, G.; Grossi, M.; Jordán, A.; Hess, K. M.; Huertas-Company, M.; Hunt, L. K.; Kent, B. R.; Lambas, D. G.; Lançon, A.; MacArthur, L. A.; Madden, S. C.; Magrini, L.; Mei, S.; Momjian, E.; Olowin, R. P.; Papastergis, E.; Smith, M. W. L.; Solanes, J. M.; Spector, O.; Spekkens, K.; Taylor, J. E.; Valotto, C.; van Driel, W.; Verstappen, J.; Vlahakis, C.; Vollmer, B.; Xilouris, E. M. (2011)The GALEX Ultraviolet Virgo Cluster Survey (GUViCS) is a complete blind survey of the Virgo cluster covering ~40 sq. deg in the far UV (FUV, ?<SUB>eff</SUB> = 1539 Å, ?? = 442 Å) and ~120 sq. deg in the near UV (NUV, ...
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Bussmann, R. S.; Riechers, D.; Fialkov, A.; Scudder, J.; Hayward, C. C.; Cowley, W. I.; Bock, J.; Calanog, J.; Chapman, S. C.; Cooray, A.; De Bernardis, F.; Farrah, D.; Fu, Hai; Gavazzi, R.; Hopwood, R.; Ivison, R. J.; Jarvis, M.; Lacey, C.; Loeb, A.; Oliver, S. J.; Pérez-Fournon, I.; Rigopoulou, D.; Roseboom, I. G.; Scott, Douglas; Smith, A. J.; Vieira, J. D.; Wang, L.; Wardlow, J. (2015)The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding of these DSFGs is hampered by the limited ...
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Wardlow, Julie L.; Cooray, Asantha; De Bernardis, Francesco; Amblard, A.; Arumugam, V.; Aussel, H.; Baker, A. J.; Béthermin, M.; Blundell, R.; Bock, J.; Boselli, A.; Bridge, C.; Buat, V.; Burgarella, D.; Bussmann, R. S.; Cabrera-Lavers, A.; Calanog, J.; Carpenter, J. M.; Casey, C. M.; Castro-Rodríguez, N.; Cava, A.; Chanial, P.; Chapin, E.; Chapman, S. C.; Clements, D. L.; Conley, A.; Cox, P.; Dowell, C. D.; Dye, S.; Eales, S.; Farrah, D.; Ferrero, P.; Franceschini, A.; Frayer, D. T.; Frazer, C.; Fu, Hai; Gavazzi, R.; Glenn, J.; González Solares, E. A.; Griffin, M.; Gurwell, M. A.; Harris, A. I.; Hatziminaoglou, E.; Hopwood, R.; Hyde, A.; Ibar, E.; Ivison, R. J.; Kim, S.; Lagache, G.; Levenson, L.; Marchetti, L.; Marsden, G.; Martinez-Navajas, P.; Negrello, M.; Neri, R.; Nguyen, H. T.; O'Halloran, B.; Oliver, S. J.; Omont, A.; Page, M. J.; Panuzzo, P.; Papageorgiou, A.; Pearson, C. P.; Pérez-Fournon, I.; Pohlen, M.; Riechers, D.; Rigopoulou, D.; Roseboom, I. G.; Rowan-Robinson, M.; Schulz, B.; Scott, D.; Scoville, N.; Seymour, N.; Shupe, D. L.; Smith, A. J.; Streblyanska, A.; Strom, A.; Symeonidis, M.; Trichas, M.; Vaccari, M.; Vieira, J. D.; Viero, M.; Wang, L.; Xu, C. K.; Yan, L.; Zemcov, M. (2013)We present a list of 13 candidate gravitationally lensed submillimeter galaxies (SMGs) from 95 deg<SUP>2</SUP> of the Herschel Multi-tiered Extragalactic Survey, a surface density of 0.14 ± 0.04 deg<SUP>-2</SUP>. The ...
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Dowell, C. Darren; Conley, A.; Glenn, J.; Arumugam, V.; Asboth, V.; Aussel, H.; Bertoldi, F.; Béthermin, M.; Bock, J.; Boselli, A.; Bridge, C.; Buat, V.; Burgarella, D.; Cabrera-Lavers, A.; Casey, C. M.; Chapman, S. C.; Clements, D. L.; Conversi, L.; Cooray, A.; Dannerbauer, H.; De Bernardis, F.; Ellsworth-Bowers, T. P.; Farrah, D.; Franceschini, A.; Griffin, M.; Gurwell, M. A.; Halpern, M.; Hatziminaoglou, E.; Heinis, S.; Ibar, E.; Ivison, R. J.; Laporte, N.; Marchetti, L.; Martínez-Navajas, P.; Marsden, G.; Morrison, G. E.; Nguyen, H. T.; O'Halloran, B.; Oliver, S. J.; Omont, A.; Page, M. J.; Papageorgiou, A.; Pearson, C. P.; Petitpas, Glen R.; Pérez-Fournon, I.; Pohlen, M.; Riechers, D.; Rigopoulou, D.; Roseboom, I. G.; Rowan-Robinson, M.; Sayers, J.; Schulz, B.; Scott, Douglas; Seymour, N.; Shupe, D. L.; Smith, A. J.; Streblyanska, A.; Symeonidis, M.; Vaccari, M.; Valtchanov, I.; Vieira, J. D.; Viero, M.; Wang, L.; Wardlow, J.; Xu, C. K.; Zemcov, M. (2014)We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral and Photometric Imaging Receiver 250/350/500 ?m flux densities to search for red sources. We apply this method to 21 ...
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Huang, J. -S; Faber, S. M.; Daddi, E.; Laird, E. S.; Lai, K.; Omont, A.; Wu, Y.; Younger, J. D.; Bundy, K.; Cattaneo, A.; Chapman, S. C.; Conselice, C. J.; Dickinson, M.; Egami, E.; Fazio, Giovanni G.; Im, M.; Koo, D.; LeFloc'h, E.; Papovich, C.; Rigopoulou, D.; Smail, I.; Song, M.; Van, de Werf; Webb, T. M. A.; Willmer, C. N. A.; Willner, Steven P.; Yan, L. (2009)
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